Fig. 6
VVV Ks-band light curve of Nova Sgr 2010b. The VVV data caught the object about 0.5 days before its first detection in eruption. The object is seen as a saturated source on 23 March 2010 and recorded about 2 mags fainter on 12 Sep. 2010. Sgr 2010b is beyond detection (Ks ≳ 16.2 mag in the VVV Ks-band aperture catalogues for this field) in a sequence of observations from Sep. 2011 to Apr. 2012.
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